Computer Science
Scientific paper
Feb 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ge%26ae..27q.109b&link_type=abstract
Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 27, Jan.-Feb. 1987, p. 109-114. In Russian.
Computer Science
Auroral Zones, Daytime, Geomagnetic Pulsations, Interplanetary Magnetic Fields, Polar Cusps, Field Aligned Currents, Spatial Distribution, Temporal Distribution
Scientific paper
It is established that Pi1C pulsations are a characteristic oscillation regime in the region of the dayside polar cusp. The characteristics of dayside Pi1C pulsations are shown to depend on IMF parameters; the latitudinal and longitudinal localization of these pulsations is determined by a specific combination of the azimuthal and vertical components of the IMF. The Pi1C pulsations are shown to be correlated with field-aligned currents in the dayside sector of the auroral oval. It is suggested that these pulsations arise as the result of fluctuations of the three-dimensional ionospheric-magnetospheric current system.
Bolshakova O. V.
Borovkova O. K.
Khorosheva O. V.
Troitskaia V. A.
No associations
LandOfFree
Pi1C pulsations in the dayside sector of the auroral oval does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Pi1C pulsations in the dayside sector of the auroral oval, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Pi1C pulsations in the dayside sector of the auroral oval will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1012255